1973
DOI: 10.1103/physrevlett.30.471
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Observation of aKX-Ray Band Emitted by the Transient C-C System Formed at keV Energies

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Cited by 59 publications
(9 citation statements)
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“…Two questions frequently encountered, are (1) are molecular orbital (MO) x rays being observed, and (2) what is the mechanism for the production of MO xrays? In this paper we consider K MO x rays, arising from transitions to vacancies in the l sa MO.…”
Section: Introductionmentioning
confidence: 99%
“…Two questions frequently encountered, are (1) are molecular orbital (MO) x rays being observed, and (2) what is the mechanism for the production of MO xrays? In this paper we consider K MO x rays, arising from transitions to vacancies in the l sa MO.…”
Section: Introductionmentioning
confidence: 99%
“…From all competing effects mentioned in Chapter 1, we suppose the quasimolecular (MO) radiation to be admixed dominantly. For the asymmetric diatomic systems considered here this radiation should arise in the target materials by adiabatic collisions between recoil atoms and atoms at rest [15]. Using the formulae given by Heinig et al [16] we constructed the correlation diagrams of the (neutral) collision systems Si + Si and Ti+Ti by scaling the H~ diagrams with state dependent screened nuclear charges.…”
Section: Discussion Of the Resultsmentioning
confidence: 99%
“…Most of these calculations 1 are based on the Born approximation for direct Coulomb ionization established by Bethe. 2 In this paper we apply the more rigorous Glauber approximation 3 to the ionization of atomic hydrogen by electron impact to compute the total cross section as a function of the energy of the incident electron.…”
Section: Calculation Of Total Cross Sections For the Ionization Of Atmentioning
confidence: 99%
“…3,5 The interpretation of experiments involving MO K x-ray emission from high-energy collisions of heavier ions with heavy atoms are presently more speculative. One of the principal difficulties in interpreting these measurements is that the available theories of inner-shell vacancy production in high-energy, heavy-ion-atom collisions are not sufficiently developed to permit prediction of the details of the spectral distribution and of the features of the production cross section such that these can be exploited as a guide for identifying MO K x-ray emission.…”
mentioning
confidence: 99%